pith. machine review for the scientific record. sign in

arxiv: 2604.08444 · v1 · submitted 2026-04-09 · ✦ hep-ph

Recognition: unknown

LFV decays in a 3-4-1 model with minimal inverse seesaw neutrinos

Authors on Pith no claims yet

Pith reviewed 2026-05-10 17:11 UTC · model grok-4.3

classification ✦ hep-ph
keywords 3-4-1 modelminimal inverse seesawlepton flavor violationmuon g-2 anomalytau to mu gammacharged Higgsneutrino masses
0
0 comments X

The pith

A 3-4-1 model with minimal inverse seesaw neutrinos generates strong correlations between the electron and muon g-2 anomalies and lepton flavor violating decay rates.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The paper studies an extended 3-4-1 gauge model that adds a new singly charged Higgs boson and implements the minimal inverse seesaw mechanism for generating neutrino masses. This construction simultaneously explains the observed anomalies in the electron and muon anomalous magnetic moments while producing lepton flavor violating decays of charged leptons, the Standard Model-like Higgs boson, and the Z boson. The central result is that the model creates tight correlations among these quantities. In particular, the present experimental upper limit on the branching fraction of tau to muon gamma decay restricts the allowed deviation in the muon g-2 to at most 10 to the minus 9 from the Standard Model value, remaining compatible with the one-sigma experimental range.

Core claim

The model predicts strong correlations among the (g-2)e,μ anomalies and the LFV decay rates of charged leptons, the SM-like Higgs, and the Z boson. The current upper bound on Br(τ → μγ) imposes a stringent constraint compatible with the 1σ experimental range of (g-2)μ, corresponding to a maximal deviation of 10^{-9} from the SM prediction. The forthcoming experimental sensitivity to Br(τ → μγ) will reduce this deviation to 5×10^{-10}.

What carries the argument

The 3-4-1 gauge symmetry extended by a minimal inverse seesaw neutrino sector and a new singly charged Higgs boson, whose Yukawa couplings and mass parameters generate the correlations between the magnetic moment anomalies and the flavor-violating processes.

If this is right

  • The existing upper limit on Br(τ → μγ) caps the maximum allowed deviation in (g-2)μ at 10^{-9}.
  • Improved sensitivity to Br(τ → μγ) will further restrict the possible (g-2)μ shift to 5×10^{-10}.
  • The same parameter choices that fit the g-2 anomalies also determine the rates for LFV decays of the Higgs and Z bosons.
  • All current experimental data on these observables can be accommodated simultaneously within the model.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • Independent searches for the new singly charged Higgs at colliders could test the same parameter region that controls the g-2 and LFV correlations.
  • The required neutrino mass matrices may imply specific patterns in oscillation data or neutrinoless double-beta decay rates.
  • If the g-2 anomalies are confirmed at the predicted level, the model would forecast measurable LFV signals at next-generation flavor experiments.

Load-bearing premise

The Yukawa couplings and mass parameters in the minimal inverse seesaw sector can be adjusted to fit the g-2 anomalies while keeping all lepton flavor violating rates below current experimental limits and consistent with observed neutrino masses.

What would settle it

A future measurement showing Br(τ → μγ) below the current bound together with a (g-2)μ deviation larger than 10^{-9} from the Standard Model value would contradict the correlations required by the model.

Figures

Figures reproduced from arXiv: 2604.08444 by L.T. Hue, L.T.T. Phuong, N.H.T. Nha, T.T. Hong.

Figure 1
Figure 1. Figure 1: FIG. 1: Feynman diagrams giving one-loop contributions to the decay [PITH_FULL_IMAGE:figures/full_fig_p011_1.png] view at source ↗
Figure 2
Figure 2. Figure 2: FIG. 2: One-loop Feynman diagrams contributing to [PITH_FULL_IMAGE:figures/full_fig_p012_2.png] view at source ↗
Figure 3
Figure 3. Figure 3: FIG. 3: Feynman diagrams for one-loop contributions to the decay amplitudes [PITH_FULL_IMAGE:figures/full_fig_p014_3.png] view at source ↗
Figure 4
Figure 4. Figure 4: FIG. 4: The correlations between ∆ [PITH_FULL_IMAGE:figures/full_fig_p017_4.png] view at source ↗
Figure 5
Figure 5. Figure 5: FIG. 5: The correlations between ∆ [PITH_FULL_IMAGE:figures/full_fig_p018_5.png] view at source ↗
Figure 6
Figure 6. Figure 6: FIG. 6: The relationship between decay rates of cLFV, LFV [PITH_FULL_IMAGE:figures/full_fig_p018_6.png] view at source ↗
read the original abstract

We investigate an extended 3-4-1 model consisting of a new singly charged Higgs boson, implementing the minimal inverse seesaw mechanism to accommodate the large values of the $(g-2)_{e,\mu}$ anomalies as well as the lepton-flavor-violating decay rates of charged leptons, the Standard Model-like Higgs boson, and the $Z$ boson, all consistent with current experimental data. Unlike the previously studied 3-4-1 realization, the model considered here predicts strong correlations among these observables that can be tested in future experiments. In particular, the current upper bound on Br$(\tau \to \mu \gamma)$ imposes a stringent constraint compatible with the $1\sigma$ experimental range of $(g-2)_{\mu}$, corresponding to a maximal deviation of $10^{-9}$ from the SM prediction. The forthcoming experimental sensitivity to Br$(\tau \to \mu\gamma)$ will reduce this deviation to $5\times 10^{-10}$.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

0 major / 2 minor

Summary. The manuscript presents a 3-4-1 gauge extension with a singly charged Higgs boson and minimal inverse seesaw neutrinos. It derives one-loop contributions to the (g-2)e,μ anomalies and to LFV processes (τ→μγ, h→τμ, Z→τμ), then performs a numerical scan over the allowed parameter space subject to neutrino oscillation data and collider bounds. The central result is a set of strong correlations among these observables, with the current experimental upper limit on Br(τ→μγ) restricting the maximal (g-2)μ deviation to 10^{-9} within the 1σ experimental range, and future sensitivity tightening this to 5×10^{-10}.

Significance. If the numerical results hold, the work supplies concrete, falsifiable correlations between the (g-2) anomalies and LFV branching ratios that can be tested at Belle II and future colliders, distinguishing this 3-4-1 realization from earlier variants. Credit is due for the explicit one-loop expressions, the imposition of neutrino-mass and collider constraints, and the quantitative mapping of the allowed region in observable space.

minor comments (2)
  1. [Section 3] Section 3 (or wherever the inverse-seesaw Yukawa matrices are introduced): explicit matrix forms for the Yukawa couplings and the small lepton-number-violating parameter would improve reproducibility of the loop integrals and mixing angles.
  2. [Numerical results] Numerical scan subsection: the ranges, priors, and sampling method for the free parameters (Yukawas, new Higgs and neutrino masses) should be stated more precisely so that the reported maximal deviations and correlation bands can be independently verified.

Simulated Author's Rebuttal

0 responses · 0 unresolved

We thank the referee for the positive assessment of our manuscript on LFV decays in the 3-4-1 model with minimal inverse seesaw neutrinos and for recommending minor revision. The referee summary correctly reflects the central predictions of strong correlations between the (g-2) anomalies and LFV rates, with the τ→μγ bound limiting the muon anomaly. No major comments were provided in the report.

Circularity Check

0 steps flagged

No significant circularity; derivation is self-contained

full rationale

The paper constructs a 3-4-1 gauge model with minimal inverse seesaw, derives one-loop contributions to (g-2)e,μ and LFV processes from explicit Feynman diagrams and mixing matrices, then performs a numerical scan over Yukawa couplings and mass parameters subject to neutrino oscillation data and collider bounds. The reported correlations and maximal (g-2)μ deviation under the Br(τ→μγ) limit emerge directly from evaluating the loop functions over the allowed parameter region; no step reduces by definition or self-citation to the target observables themselves. The central claim is therefore a genuine model prediction rather than a re-expression of fitted inputs.

Axiom & Free-Parameter Ledger

2 free parameters · 2 axioms · 1 invented entities

The central claim depends on several fitted parameters in the scalar and fermion sectors to match the experimental anomalies, plus standard assumptions of the seesaw mechanism.

free parameters (2)
  • Yukawa couplings in inverse seesaw
    Adjusted to fit (g-2) anomalies and LFV rates
  • Masses of new Higgs and neutrinos
    Chosen to accommodate large (g-2) values while satisfying bounds
axioms (2)
  • domain assumption The 3-4-1 gauge symmetry and particle content
    Standard extension assumed as the base model
  • domain assumption Minimal inverse seesaw mechanism generates small neutrino masses
    Used to explain neutrino masses and contribute to anomalies
invented entities (1)
  • Singly charged Higgs boson no independent evidence
    purpose: Mediates contributions to (g-2) and LFV decays
    New particle postulated in the model to achieve the desired phenomenology

pith-pipeline@v0.9.0 · 5482 in / 1709 out tokens · 77410 ms · 2026-05-10T17:11:06.357173+00:00 · methodology

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Reference graph

Works this paper leans on

94 extracted references · 90 canonical work pages

  1. [1]

    In the limitµ X → O 2×2, the rankM ν reduces from 6 to 4, which will leave three light neutrinos massless, which exactly matches the SM. The most significant aspect of mISS is that it predicts that the lightest neutrino is exactly massless because the Dirac mass matrixm D is 3×2 matrix have rank 2, which differs from the original ISS. Hence,m n1(n3) = 0 f...

  2. [2]

    R. Foot, H. N. Long and T. A. Tran, Phys. Rev. D50(1994) no.1, R34-R38 [arXiv:hep- ph/9402243 [hep-ph]]. 25

  3. [3]

    Pisano and V

    F. Pisano and V. Pleitez, Phys. Rev. D51(1995), 3865-3869 [arXiv:hep-ph/9401272 [hep-ph]]

  4. [4]

    M. B. Voloshin, Sov. J. Nucl. Phys.48(1988), 512 ITEP-87-215

  5. [5]

    W. A. Ponce, D. A. Gutierrez and L. A. Sanchez, Phys. Rev. D69(2004), 055007 [arXiv:hep- ph/0312143 [hep-ph]]

  6. [6]

    L. A. Sanchez, F. A. Perez and W. A. Ponce, Eur. Phys. J. C35(2004), 259-265 [arXiv:hep- ph/0404005 [hep-ph]]

  7. [7]

    W. A. Ponce and L. A. Sanchez, Mod. Phys. Lett. A22(2007), 435-448 [arXiv:hep-ph/0607175 [hep-ph]]

  8. [8]

    L. A. Sanchez, L. A. Wills-Toro and J. I. Zuluaga, Phys. Rev. D77(2008), 035008 [arXiv:0801.4044 [hep-ph]]

  9. [9]

    Riazuddin and Fayyazuddin, Eur. Phys. J. C56(2008), 389-394 [arXiv:0803.4267 [hep-ph]]

  10. [10]

    S. h. Nam, K. Y. Lee and Y. Y. Keum, Phys. Rev. D82(2010), 105027 [arXiv:0909.3770 [hep-ph]]

  11. [11]

    Palacio, Int

    G. Palacio, Int. J. Mod. Phys. A31(2016) no.25, 1650142 [arXiv:1608.08676 [hep-ph]]

  12. [12]

    H. N. Long, L. T. Hue and D. V. Loi, Phys. Rev. D94(2016) no.1, 015007 [arXiv:1605.07835 [hep-ph]]

  13. [13]

    Djouala, N

    M. Djouala, N. Mebarki and H. Aissaoui, Int. J. Mod. Phys. A36(2021) no.17, 17 [arXiv:1911.04887 [hep-ph]]

  14. [14]

    Cogollo, Y

    D. Cogollo, Y. M. Oviedo-Torres and Y. S. Villamizar, Int. J. Mod. Phys. A35(2020) no.23, 2050126 [arXiv:2004.14792 [hep-ph]]

  15. [15]

    N. H. Thao, D. T. Binh, T. T. Hong, L. T. Hue and D. P. Khoi, PTEP2023, no.8, 083B02 (2023) doi:10.1093/ptep/ptad092 [arXiv:2302.07576 [hep-ph]]

  16. [16]

    D. P. Aguillardet al.[Muon g-2], Phys. Rev. Lett.131(2023) no.16, 161802 [arXiv:2308.06230 [hep-ex]]

  17. [17]

    D. P. Aguillardet al.[Muon g-2], Phys. Rev. Lett.135(2025) no.10, 101802 [arXiv:2506.03069 [hep-ex]]

  18. [18]

    Aliberti, T

    R. Aliberti, T. Aoyama, E. Balzani, A. Bashir, G. Benton, J. Bijnens, V. Biloshyt- skyi, T. Blum, D. Boito and M. Bruno,et al.Phys. Rept.1143, 1-158 (2025) doi:10.1016/j.physrep.2025.08.002 [arXiv:2505.21476 [hep-ph]]

  19. [19]

    D. W. Hertzog and M. Hoferichter, [arXiv:2512.16980 [hep-ph]]

  20. [20]

    Athron, K

    P. Athron, K. M¨ ohling, D. St¨ ockinger and H. St¨ ockinger-Kim, Prog. Part. Nucl. Phys.148 26 (2026), 104225 [arXiv:2507.09289 [hep-ph]]

  21. [21]

    M. W. Li, X. G. He, A. Cheek and X. Chu, Phys. Lett. B871, 139949 (2025) doi:10.1016/j.physletb.2025.139949 [arXiv:2506.05511 [hep-ph]]

  22. [22]

    Hanneke, S

    D. Hanneke, S. Fogwell and G. Gabrielse, Phys. Rev. Lett.100(2008), 120801 [arXiv:0801.1134 [physics.atom-ph]]

  23. [23]

    R. H. Parker, C. Yu, W. Zhong, B. Estey and H. M¨ uller, Science360(2018), 191 doi:10.1126/science.aap7706 [arXiv:1812.04130 [physics.atom-ph]]

  24. [24]

    Morel, Z

    L. Morel, Z. Yao, P. Clad´ e and S. Guellati-Kh´ elifa, Nature588(2020) no.7836, 61-65 doi:10.1038/s41586-020-2964-7

  25. [25]

    X. Fan, T. G. Myers, B. A. D. Sukra and G. Gabrielse, Phys. Rev. Lett.130(2023) no.7, 071801 doi:10.1103/PhysRevLett.130.071801 [arXiv:2209.13084 [physics.atom-ph]]

  26. [26]

    Aoyama, M

    T. Aoyama, M. Hayakawa, T. Kinoshita and M. Nio, Phys. Rev. Lett.109(2012), 111807 doi:10.1103/PhysRevLett.109.111807 [arXiv:1205.5368 [hep-ph]]

  27. [27]

    Laporta, Phys

    S. Laporta, Phys. Lett. B772(2017), 232-238 doi:10.1016/j.physletb.2017.06.056 [arXiv:1704.06996 [hep-ph]]

  28. [28]

    Aoyama, T

    T. Aoyama, T. Kinoshita and M. Nio, Phys. Rev. D97(2018) no.3, 036001 doi:10.1103/PhysRevD.97.036001 [arXiv:1712.06060 [hep-ph]]. [28]

  29. [29]

    Volkov, Phys

    S. Volkov, Phys. Rev. D100(2019) no.9, 096004 doi:10.1103/PhysRevD.100.096004 [arXiv:1909.08015 [hep-ph]]

  30. [30]

    X. F. Han, T. Li, L. Wang and Y. Zhang, Phys. Rev. D99(2019) no.9, 095034 [arXiv:1812.02449 [hep-ph]]

  31. [31]

    Endo and W

    M. Endo and W. Yin, JHEP08(2019), 122 [arXiv:1906.08768 [hep-ph]]

  32. [32]

    E. J. Chun and T. Mondal, JHEP11(2020), 077 [arXiv:2009.08314 [hep-ph]]

  33. [33]

    Delle Rose, S

    L. Delle Rose, S. Khalil and S. Moretti, Phys. Lett. B816(2021), 136216 [arXiv:2012.06911 [hep-ph]]

  34. [34]

    F. J. Botella, F. Cornet-Gomez and M. Nebot, Phys. Rev. D102(2020) no.3, 035023 [arXiv:2006.01934 [hep-ph]]

  35. [35]

    S. P. Li, X. Q. Li, Y. Y. Li, Y. D. Yang and X. Zhang, JHEP01(2021), 034 [arXiv:2010.02799 [hep-ph]]

  36. [36]

    Bigaran and R

    I. Bigaran and R. R. Volkas, Phys. Rev. D102(2020) no.7, 075037 27 doi:10.1103/PhysRevD.102.075037 [arXiv:2002.12544 [hep-ph]]

  37. [37]

    X. F. Han, T. Li, H. X. Wang, L. Wang and Y. Zhang, Phys. Rev. D104(2021) no.11, 115001 [arXiv:2104.03227 [hep-ph]]

  38. [38]

    Bharadwaj, S

    H. Bharadwaj, S. Dutta and A. Goyal, JHEP11(2021), 056 [arXiv:2109.02586 [hep-ph]]

  39. [39]

    Arbel´ aez, R

    C. Arbel´ aez, R. Cepedello, R. M. Fonseca and M. Hirsch, Phys. Rev. D102(2020) no.7, 075005 [arXiv:2007.11007 [hep-ph]]

  40. [40]

    K. F. Chen, C. W. Chiang and K. Yagyu, JHEP09(2020), 119 [arXiv:2006.07929 [hep-ph]]

  41. [41]

    Dutta, S

    B. Dutta, S. Ghosh and T. Li, Phys. Rev. D102(2020) no.5, 055017 [arXiv:2006.01319 [hep-ph]]

  42. [42]

    A. E. C. Hern´ andez, S. F. King and H. Lee, Phys. Rev. D103(2021) no.11, 115024 [arXiv:2101.05819 [hep-ph]]

  43. [43]

    A. E. C. Hern´ andez, D. T. Huong and I. Schmidt, Eur. Phys. J. C82(2022) no.1, 63 [arXiv:2109.12118 [hep-ph]]

  44. [44]

    S. Li, Z. Li, F. Wang and J. M. Yang, Nucl. Phys. B983(2022), 115927 [arXiv:2205.15153 [hep-ph]]

  45. [45]

    F. J. Botella, F. Cornet-Gomez, C. Mir´ o and M. Nebot, Eur. Phys. J. C82(2022), 915 [arXiv:2205.01115 [hep-ph]]

  46. [46]

    L. Wang, J. M. Yang and Y. Zhang, Commun. Theor. Phys.74(2022) no.9, 097202 [arXiv:2203.07244 [hep-ph]]

  47. [47]

    Kriewald, J

    J. Kriewald, J. Orloff, E. Pinsard and A. M. Teixeira, Eur. Phys. J. C82(2022) no.9, 844 [arXiv:2204.13134 [hep-ph]]

  48. [48]

    R. K. Barman, R. Dcruz and A. Thapa, JHEP03(2022), 183 [arXiv:2112.04523 [hep-ph]]

  49. [49]

    Dermisek, Moscow Univ

    R. Dermisek, Moscow Univ. Phys. Bull.77(2022) no.2, 102-107 [arXiv:2201.06179 [hep-ph]]

  50. [50]

    T. A. Chowdhury, M. Ehsanuzzaman and S. Saad, JCAP08(2022), 076 [arXiv:2203.14983 [hep-ph]]

  51. [51]

    C. H. Chen, C. W. Chiang and C. W. Su, J. Phys. G51(2024) no.8, 085001 [arXiv:2301.07070 [hep-ph]]

  52. [52]

    Navaset al.[Particle Data Group], Phys

    S. Navaset al.[Particle Data Group], Phys. Rev. D110, no.3, 030001 (2024) doi:10.1103/PhysRevD.110.030001

  53. [53]

    Venturini [MEG II], Nuovo Cim

    A. Venturini [MEG II], Nuovo Cim. C47, no.5, 287 (2024) doi:10.1393/ncc/i2024-24287-4

  54. [54]

    Afanacievet al.[MEG II], Eur

    K. Afanacievet al.[MEG II], Eur. Phys. J. C85, no.10, 1177 (2025) [erratum: Eur. Phys. J. 28 C85, no.11, 1317 (2025)] doi:10.1140/epjc/s10052-025-14906-3 [arXiv:2504.15711 [hep-ex]]

  55. [55]

    A. M. Baldiniet al.[MEG II], Eur. Phys. J. C78(2018) no.5, 380 [arXiv:1801.04688 [physics.ins-det]]

  56. [56]

    Ferber,Towards First Physics at Belle II,Acta Phys

    E. Kouet al.[Belle-II], PTEP2019(2019) no.12, 123C01 [erratum: PTEP2020(2020) no.2, 029201] [arXiv:1808.10567 [hep-ex]]

  57. [57]

    Aubert et al

    B. Aubertet al.[BaBar], Phys. Rev. Lett.104(2010), 021802 [arXiv:0908.2381 [hep-ex]]

  58. [58]

    A. M. Baldiniet al.[MEG], Eur. Phys. J. C76(2016) no.8, 434 [arXiv:1605.05081 [hep-ex]]

  59. [59]

    Abdesselam et al

    A. Abdesselamet al.[Belle], JHEP10(2021), 19 [arXiv:2103.12994 [hep-ex]]

  60. [60]

    Q. Qin, Q. Li, C. D. L¨ u, F. S. Yu and S. H. Zhou, Eur. Phys. J. C78, no.10, 835 (2018) [arXiv:1711.07243 [hep-ph]]

  61. [61]

    A. M. Sirunyanet al.[CMS], Phys. Rev. D104, no.3, 032013 (2021) [arXiv:2105.03007 [hep- ex]]

  62. [62]

    R. K. Barman, P. S. B. Dev and A. Thapa, Phys. Rev. D107, no.7, 075018 (2023) doi:10.1103/PhysRevD.107.075018 [arXiv:2210.16287 [hep-ph]]

  63. [63]

    M. Aoki, S. Kanemura, M. Takeuchi and L. Zamakhsyari, Phys. Rev. D107, no.5, 055037 (2023) doi:10.1103/PhysRevD.107.055037 [arXiv:2302.08489 [hep-ph]]

  64. [64]

    Aadet al.[ATLAS], Phys

    G. Aadet al.[ATLAS], Phys. Rev. D108, 032015 (2023) doi:10.1103/PhysRevD.108.032015 [arXiv:2204.10783 [hep-ex]]

  65. [65]

    Aadet al.[ATLAS], Phys

    G. Aadet al.[ATLAS], Phys. Rev. Lett.127, 271801 (2022) doi:10.1103/PhysRevLett.127.271801 [arXiv:2105.12491 [hep-ex]]

  66. [66]

    Dam, SciPost Phys

    M. Dam, SciPost Phys. Proc.1, 041 (2019) doi:10.21468/SciPostPhysProc.1.041 [arXiv:1811.09408 [hep-ex]]

  67. [67]

    Abadaet al.[FCC], Eur

    A. Abadaet al.[FCC], Eur. Phys. J. C79, no.6, 474 (2019) doi:10.1140/epjc/s10052-019- 6904-3

  68. [68]

    Malinsky, T

    M. Malinsky, T. Ohlsson, Z. z. Xing and H. Zhang, Phys. Lett. B679, 242-248 (2009) doi:10.1016/j.physletb.2009.07.038 [arXiv:0905.2889 [hep-ph]]

  69. [69]

    J. A. Casas and A. Ibarra, Nucl. Phys. B618, 171-204 (2001) doi:10.1016/S0550- 3213(01)00475-8 [arXiv:hep-ph/0103065 [hep-ph]]

  70. [70]

    Pontecorvo, Sov

    B. Pontecorvo, Sov. Phys. JETP6, 429-431 (1958)

  71. [71]

    Z. Maki, M. Nakagawa and S. Sakata, Prog. Theor. Phys.28, 870-880 (1962) doi:10.1143/PTP.28.870 29

  72. [72]

    Arganda, M

    E. Arganda, M. J. Herrero, X. Marcano and C. Weiland, Phys. Rev. D91, no.1, 015001 (2015) doi:10.1103/PhysRevD.91.015001 [arXiv:1405.4300 [hep-ph]]

  73. [73]

    N. H. Thao, L. T. Hue, H. T. Hung and N. T. Xuan, Nucl. Phys. B921, 159-180 (2017) doi:10.1016/j.nuclphysb.2017.05.014 [arXiv:1703.00896 [hep-ph]]

  74. [74]

    T. T. Hong, L. T. T. Phuong, T. P. Nguyen, N. H. T. Nha and L. T. Hue, Phys. Rev. D110, no.7, 075010 (2024) doi:10.1103/PhysRevD.110.075010 [arXiv:2404.05524 [hep-ph]]

  75. [75]

    L. T. Hue, K. H. Phan, T. T. Hong, T. P. Nguyen and N. H. T. Nha, Eur. Phys. J. C84 (2024) no.12, 1262 [arXiv:2409.01390 [hep-ph]]

  76. [76]

    Arganda, A

    E. Arganda, A. M. Curiel, M. J. Herrero and D. Temes, Phys. Rev. D71, 035011 (2005) doi:10.1103/PhysRevD.71.035011 [arXiv:hep-ph/0407302 [hep-ph]]

  77. [77]

    T. T. Hong, N. H. T. Nha, T. P. Nguyen, L. T. T. Phuong and L. T. Hue, PTEP2022(2022) no.9, 093B05 [arXiv:2206.08028 [hep-ph]]

  78. [78]

    T. P. Nguyen, T. T. Le, T. T. Hong and L. T. Hue, Phys. Rev. D97, no.7, 073003 (2018) doi:10.1103/PhysRevD.97.073003 [arXiv:1802.00429 [hep-ph]]

  79. [79]

    Denner, S

    A. Denner, S. Heinemeyer, I. Puljak, D. Rebuzzi and M. Spira, Eur. Phys. J. C71, 1753 (2011) doi:10.1140/epjc/s10052-011-1753-8 [arXiv:1107.5909 [hep-ph]]

  80. [80]

    Jurˇ ciukonis and L

    D. Jurˇ ciukonis and L. Lavoura, JHEP03, 106 (2022) doi:10.1007/JHEP03(2022)106 [arXiv:2107.14207 [hep-ph]]

Showing first 80 references.